Using the data set from T-239 to T+963 s from recent telemetry
downlinks, we report that this is a very weak source in BAT,
and as such a description of the mask-weighted light curve is
problematic.
The time-averaged spectrum from T+0.0 to T+376 s is best fit
by a simple power-law model with a photon index of 3.18 +/- 0.78.
The fluence (same time interval) in the 15-150 keV band is
(4.4 +/- 1.6)E-7 erg cm-2. All quoted errors are at the 90% c.l.

The XRT began observing the field at 14:25:34.6 UT, 452 s after
the BAT trigger. The XRT light curve shows the descending part
of a flare that reached about 4 counts s-1.
The mean XRT/PC spectrum (T+461 to 1025 s) can be fit by an
absorbed power-law model with a photon index of 0.7+/-0.6
and an absorbing column density of NH=(6+3-2)E22 cm-2.
The average 0.3-10 keV observed (unabsorbed) flux is
3.5E-10 (4.7E-10) erg cm-2 s-1.